Scientists used computer simulations to predict weather conditions on the K2-141b.
On the "night" side, the temperature drops to-200 ° C. The "daytime" half of the exoplanet heats up to 3000 ° C. This high temperature not only melts rocks on the planet's surface, but also vaporizes them, eventually creating a thin "rock atmosphere".
It is noteworthy that the atmosphere of stone steam,created due to extreme heat is subject to precipitation. Similar to the Earth's water cycle - when it evaporates, rises into the atmosphere, condenses and falls back as rain - the same happens with sodium, silicon monoxide and silicon dioxide on K2-141b. On Earth, rain falls back into the oceans, where it evaporates again. On K2-141b, the mineral vapor is carried away by supersonic winds to the cold "night" side, where rocks "rain" down into the magma ocean. The streams again end up on the hot side of the exoplanet, where the rocks evaporate again.
“All rocky planets, including the Earth,started out as molten worlds, but then quickly cooled and solidified. The lava planets give us a rare glimpse into this stage of planetary evolution, ”said Professor Cowan of the Department of Earth and Planetary Sciences at McGill University.
The next step of scientists will be to checkthe correctness of these predictions. Researchers now have data from the Spitzer Space Telescope that will give them their first idea of the exoplanet's actual day and night temperatures. With the launch of the James Webb Space Telescope in 2021, they will also be able to check if the weather on K2-141b matches scientists' predictions.
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